The most promising astrophysical sources of kHz gravitational waves (GWs) are the inspiral
and merger of binary neutron star (NS)/black hole systems. Maximizing the scientific return …

This is a new review covering developments in 'atomic spectrometry'. It combines the content
of the previously separate ASU reviews on 'atomic emission, absorption and fluorescence …

During the past 20 years, part of our work has been focused on the study of the atomic
structure and the determination of radiative parameters in neutral and slightly ionized heavy …

Context. The sharp-line spectrum of the non-magnetic, main-sequence Bp star HR 6000 has
peculiarities that distinguish it from those of the HgMn stars with which it is sometimes …

Aims. It is now well established that a large amount of heavy (trans-iron) elements are
produced during neutron star (NS) mergers. These elements can be detected in the spectra …

Landé g-factors are calculated, in intermediate coupling, for 2084 levels belonging to atoms
or ions of the sixth row of the periodic table. Extensive configuration interaction and …

Experimental relative transition probabilities for the 16 more pro-eminent lines arising from
the 6p configurations of Au II were determined from the emission-line intensities in a laser …

Abundance observations indicate the presence of rapid-neutron capture (ie, r-process)
elements in old Galactic halo and globular cluster stars. Recent observations of the r …

The references cited in this section are mostly papers on original laboratory research;
compilations and data bases are covered in another section. The references, ordered by …

The present paper is an update and extension of previous compilations [1, 2] and it
describes recent progress regarding the investigation of the radiative properties of the …